| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.37 | 139.53 | 23.94 | 176.16 | -19.26 | 335.46 | -64.17 | 112.54 | 0.9163 | 401.4 | 132.6 | |
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back to the solar disc SDO HMI 2011-11-13 06:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.70 | 111.04 | 18.36 | 122.20 | -17.79 | 339.03 | -60.60 | 111.71 | 0.8948 | 695.9 | 218.1 | |
| 0.26 | -1.00 | 0.29 | -1.00 | -17.75 | 338.67 | -60.96 | 111.57 | 0.8973 | -70.3 | 999999 | |
| 0.00 | 1.89 | 0.00 | 2.25 | -17.99 | 336.85 | -62.78 | 111.43 | 0.9104 | 372.0 | 295.5 | |
| 0.00 | 1.29 | 0.00 | 1.55 | -17.57 | 336.50 | -63.14 | 110.89 | 0.9121 | 286.0 | 189.3 | |
| 0.00 | 1.21 | 0.00 | 1.45 | -17.45 | 336.36 | -63.27 | 110.74 | 0.9128 | 168.0 | 136.9 | |
| 0.00 | 0.86 | 0.00 | 1.41 | -22.28 | 330.09 | -69.55 | 114.55 | 0.9545 | -377.0 | -349.4 | |
| 0.00 | 0.77 | 0.00 | 1.39 | -22.95 | 328.52 | -71.11 | 114.95 | 0.9622 | -304.0 | -272.9 | |
| 1.98 | 3.10 | 4.34 | 6.77 | -24.45 | 325.49 | -74.14 | 115.98 | 0.9751 | 305.7 | 67.0 | |
| 0.43 | 8.52 | 0.95 | 18.67 | -23.90 | 325.28 | -74.35 | 115.40 | 0.9755 | 197.6 | 59.0 | |
| 0.00 | 1.21 | 0.00 | 2.25 | -22.15 | 327.68 | -71.96 | 113.99 | 0.9651 | -133.0 | -63.6 | |
| 0.00 | 4.30 | 0.00 | 7.92 | -21.94 | 327.83 | -71.81 | 113.81 | 0.9643 | -547.0 | -357.8 | |
| 0.00 | 1.29 | 0.00 | 2.85 | -23.48 | 325.22 | -74.41 | 114.96 | 0.9755 | 132.0 | 137.2 | |
| 0.00 | 4.05 | 0.00 | 7.45 | -21.59 | 327.74 | -71.89 | 113.43 | 0.9644 | -173.0 | -176.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |